![Page 1: Alluvial Fan Environments Badwater Fan, Death Valley Mars](https://reader036.vdocuments.site/reader036/viewer/2022062409/5697c0271a28abf838cd6189/html5/thumbnails/1.jpg)
Alluvial Fan Environments
Badwater Fan, Death ValleyMars
![Page 2: Alluvial Fan Environments Badwater Fan, Death Valley Mars](https://reader036.vdocuments.site/reader036/viewer/2022062409/5697c0271a28abf838cd6189/html5/thumbnails/2.jpg)
Water flow nearly always supercritical on fans
Supercritical flow
Subcritical
Distinct break in gradient separates fans (steeper) from rivers (shallower)
Alluvial fans characterized by different hydrodynamic processes and resulting facies than rivers
Alluvial fans vs. rivers
![Page 3: Alluvial Fan Environments Badwater Fan, Death Valley Mars](https://reader036.vdocuments.site/reader036/viewer/2022062409/5697c0271a28abf838cd6189/html5/thumbnails/3.jpg)
Some alluvial fans, especially larger low-gradient fans, are dominated by deposits from hyperconcentrated flows and from sheetflow
Alluvial fan sediments
![Page 4: Alluvial Fan Environments Badwater Fan, Death Valley Mars](https://reader036.vdocuments.site/reader036/viewer/2022062409/5697c0271a28abf838cd6189/html5/thumbnails/4.jpg)
Miocene sheetflood deposits, Fish Canyon, California
Hyperconcentrated flow
Turbulence creates erosive base
Usually clast-supported, imbricated
Crude normal grading from unhindered settling of grains in turbulent flow
Differs from braided fluvial system by lack of
downstream accretion elements and bar forms
![Page 5: Alluvial Fan Environments Badwater Fan, Death Valley Mars](https://reader036.vdocuments.site/reader036/viewer/2022062409/5697c0271a28abf838cd6189/html5/thumbnails/5.jpg)
Smaller alluvial fans with higher relief tend to be dominated by deposition from debris flows
Active depositional lobe occasionally shifts laterally to produce fan-shaped cone of sediment
Alluvial fan sediments
![Page 6: Alluvial Fan Environments Badwater Fan, Death Valley Mars](https://reader036.vdocuments.site/reader036/viewer/2022062409/5697c0271a28abf838cd6189/html5/thumbnails/6.jpg)
Debris flows are a type of sediment gravity flow (a mixture of water and sediment particles transported by gravity without help from moving ambient water)
Sediment gravity flows classified on basis of (1) rheology and (2) sediment-support mechanism
![Page 7: Alluvial Fan Environments Badwater Fan, Death Valley Mars](https://reader036.vdocuments.site/reader036/viewer/2022062409/5697c0271a28abf838cd6189/html5/thumbnails/7.jpg)
t = m du/dyFor a Newtonian fluid like water,
Flow rheologyRheology describes the deformation of a fluid under a given shear stress
Where m is the fluid viscosity
![Page 8: Alluvial Fan Environments Badwater Fan, Death Valley Mars](https://reader036.vdocuments.site/reader036/viewer/2022062409/5697c0271a28abf838cd6189/html5/thumbnails/8.jpg)
Flow rheologyDebris flows have a plastic rheology, with a yield strength
Yield strength means that the flow will not move or deform until a certain stress has been applied
Viscosity m also constant for debris flow of given compositiont = k + m du/dy
![Page 9: Alluvial Fan Environments Badwater Fan, Death Valley Mars](https://reader036.vdocuments.site/reader036/viewer/2022062409/5697c0271a28abf838cd6189/html5/thumbnails/9.jpg)
Shear stress < yield strength causes central part of flow to move as solid plug
Friction from interaction of moving flow with the ground (and air) creates shear stress at base and top of flow
Laminar flow (due to high viscosity) where shear stress > yield strength
When driving force from gravity is too low (i.e. slope too gentle), shear stress drops below yield strength and flow “freezes” in place
![Page 10: Alluvial Fan Environments Badwater Fan, Death Valley Mars](https://reader036.vdocuments.site/reader036/viewer/2022062409/5697c0271a28abf838cd6189/html5/thumbnails/10.jpg)
How can debris flows carry such large boulders?
What forces act on boulder in debris flow?
Gravity: 4/3 p D3 rs g
Buoyancy: 4/3 p D3 rm g
Matrix Strength: Z k p D2
D, rs rm
k
Sediment-support mechanism
![Page 11: Alluvial Fan Environments Badwater Fan, Death Valley Mars](https://reader036.vdocuments.site/reader036/viewer/2022062409/5697c0271a28abf838cd6189/html5/thumbnails/11.jpg)
Gravity: 4/3 p D3 rs g
Buoyancy: 4/3 p D3 rm g
Matrix Strength: Z k p D2
D, rs rm
kMatrix density (rm) can be high (as much as 2 g/cm3, compared to 2.7-3.0 g/cm3 for rocks) due to the high sediment concentration
Weight of overlying
sediment+water
Pressure gradient
Upward force on particles
Additional buoyancy contribution in sediment-rich mixtures:
![Page 12: Alluvial Fan Environments Badwater Fan, Death Valley Mars](https://reader036.vdocuments.site/reader036/viewer/2022062409/5697c0271a28abf838cd6189/html5/thumbnails/12.jpg)
Debris flows can have high yield strength k – even large boulders do not exert sufficient shear stress on fluid to overcome k
What gives a debris flow matrix strength?
Clay minerals form network by electrostatic or atomic forces
Matrix strength a function of clay content (possible at only 2-4% clay)
Gravity: 4/3 p D3 rs g
Buoyancy: 4/3 p D3 rm g
Matrix Strength: Z k p D2
D, rs rm
k
![Page 13: Alluvial Fan Environments Badwater Fan, Death Valley Mars](https://reader036.vdocuments.site/reader036/viewer/2022062409/5697c0271a28abf838cd6189/html5/thumbnails/13.jpg)
Holocene debris flow deposits Baños, Ecuador